Evidence for the role of proton shell closure in quasi-fission reactions from X-ray fluorescence of mass-identified fragments

Evidence for the role of proton shell closure in quasi-fission reactions from X-ray fluorescence of mass-identified fragments

M. Morjean morjean@ganil.fr GANIL, CEA/DRF and CNRS/IN2P3, B.P. 55027, F-14076 Caen Cedex, France    D.J. Hinde Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    C. Simenel Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    D.Y. Jeung Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    M. Airiau Institut de Physique Nucléaire, CNRS-IN2P3, Université Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, France Irfu, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France    K.J. Cook Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    M. Dasgupta Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    A. Drouart Irfu, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France    D. Jacquet Institut de Physique Nucléaire, CNRS-IN2P3, Université Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, France    S. Kalkal [ Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    C.S. Palshetkar [ Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    E. Prasad [ Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    D. Rafferty Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    E.C. Simpson Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    L. Tassan-Got Institut de Physique Nucléaire, CNRS-IN2P3, Université Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, France    K. Vo-Phuoc Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia    E. Williams Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, ACT 0200, Australia

The atomic numbers and the masses of fragments formed in quasi-fission reactions have been simultaneously measured at scission in Ti + U reactions at a laboratory energy of 286 MeV. The atomic numbers were determined from measured characteristic fluorescence X-rays whereas the masses were obtained from the emission angles and times of flight of the two emerging fragments. For the first time, thanks to this full identification of the quasi-fission fragments on a broad angular range, the important role of the proton shell closure at Z = 82 is evidenced by the associated maximum production yield, a maximum predicted by time dependent Hartree-Fock calculations. This new experimental approach gives now access to precise studies of the time dependence of the N/Z (neutron over proton ratios of the fragments) evolution in quasi-fission reactions.

25.70.Jj, 25.70.Gh, 32.50.+d, 24.10.Cn

Present address: ] Thapar University, Patiala, Punjab 147004, India

Present address: ] Nuclear Physics Division, Bhabha Atomic Research Centre, Mumbai 400085, India.

Present address: ] Department of Physics, School of Mathematical and Physical Sciences, Central University of Kerala, Kasaragod 671314, India

Since the mid-70s, it has been known that the formation of super-heavy nuclei by fusion is hindered by out-of-equilibrium mechanisms Peter et al. (1975); Bock et al. (1982); Toke et al. (1985). In these mechanisms, the available kinetic energy can be totally dissipated and large mass transfers between the projectile and the target can occur, leading to emerging fragments quite difficult to distinguish from fragments arising from fusion followed by fission (that might be mass symmetric or asymmetric) Back (1985); Morjean et al. (2008); Frégeau et al. (2012); Jacquet and Morjean (2009). Due to these characteristics, the generic name quasi-fission (QF) is nowadays often used for all these mechanisms. Since the pioneering works, many experimental aspects of QF have been explored Materna et al. (2004); Berriman et al. (2001); Hinde et al. (2008a, b); Nishio et al. (2012); du Rietz et al. (2013); Williams et al. (2013); Wakhle et al. (2014); Kozulin et al. (2016); Prasad et al. (2016) and dynamical models, macroscopic or microscopic, have been developed in order to reproduce cross-sections, distributions of mass, angle, kinetic or excitation energy and some of the correlations between these observables Wakhle et al. (2014); Sekizawa and Yabana (2016); Li et al. (2016); Oberacker et al. (2014); *uma15; *uma16; Simenel et al. (2012); Simenel (2012); Diaz-Torres et al. (2001); Zagrebaev and Greiner (2007); Aritomo et al. (2012). Considering the huge experimental difficulties to extract in a non-arbitrary way small cross-sections of fusion followed by fission from dominant quasi-fission cross-sections, a key issue for super-heavy nucleus formation studies, it is now essential to get a very good understanding of the QF mechanisms and to confront and improve the models with unambiguous exclusive data in order to reach reliable predictive capacities.

A simultaneous determination of the fragment atomic number (Z) and mass (A) formed in QF or in fission processes remains nowadays a challenge Enqvist et al. (2001); Armbruster et al. (2004); Caamaño et al. (2013); Martin et al. (2015); Chebboubi et al. (2016), especially difficult because these quantities are most of the time measured after particle evaporation. In this letter, an experimental approach giving access for QF fragments to A and Z at scission will be presented and the data compared with predictions of a microscopic time dependent Hatree-Fock (TDHF) model Simenel (2012). The atomic number was determined from the coincident characteristic fluorescence X-rays, as already attempted for fission fragments Griffin (1990), whereas the mass was determined from the velocities of the emerging fragments.

A Ti beam was accelerated at 5.75 MeV/nucleon by the Australian National University electrostatic accelerator followed by its LINAC post-accelerator. It bombarded UF targets highly enriched in U on thin carbon or aluminum backings. Due to damage resulting from the beam impact, the targets were rapidly drilled and different sample thicknesses, ranging from 340 up to 940 , have been used during 3 days of data acquisition with a beam intensity I nA. For binary reactions, a very large range of folding angles between the 2 emerging fragments was covered by 2 large area position sensitive multi-wire proportional counters (280*360 mm) MWPC1 and MWPC2. They were positioned on opposite sides of the beam at and mm from the target, covering the angular ranges and , respectively. Coincident photons were detected by three planar germanium detectors (500 mm, 1 cm thick each) located at 6 cm from the target. These detectors were positioned at the same polar angle , but at different azimuthal angles 90, 330 and 210 with respect to the plane containing the target and the MWPC centers.

Figure 1: Photon energy spectrum for fragments with A. The red line is a fit to the data (see text).

An absolute time calibration could be achieved with a precision better than 200 ps thanks to the kinematical correlation between the detection angles and the velocities for elastically scattered projectile and target nuclei detected on broad angular ranges. A variance amu has been inferred for the mass resolution from a dedicated measurement at 3.5 MeV/nucleon, an energy much below the Coulomb barrier in which only projectile and target nuclei could be detected. With this resolution, the average masses are quite accurately determined since, from the gaussian mass distributions measured at 5.75 MeV/nucleon for elastic and weakly inelastic reactions, the actual projectile and target masses are obtained with a precision better than amu over the whole angular range. For the germanium detectors, an energy resolution eV is achieved after Doppler correction in the whole energy range involved, resulting essentially from the aperture of the germanium detectors that precludes more accurate corrections.

Figure 1 shows the photon energy spectrum for heavy fragments with A. Uranium characteristic K X-rays and the -ray at 103.5 keV from the uranium transition can be easily identified. The red line is a fit to the data with 6 gaussian distributions. The centroid, variance and normalization factor of each of the 6 distributions were free parameters in this fit. The 6 centroids found by the best fit differ by less than 100 eV from the tabulated energies either for the transition or for K X-rays from U ions (referred to in the literature as diagram rays) Kortright and Thomson (2009). Furthermore, the yield ratios between the different K transitions agree within less than 5 with the tabulated ones Kortright and Thomson (2009). Both these energies and yield ratios point out that, for the relatively low ionization states involved for the transiently formed unified atoms as well as for the emerging uranium nuclei, the relative populations on the L and M sub-shells are not sensitively modified by the processes responsible for K vacancy creation. Therefore, since on an atomic scale elastic scattering at large angles and very central nuclear reactions correspond to the same impact parameter, the emerging QF fragments should also behave for K X-ray emission like 1 ions, as already stressed in Behncke et al. (1979).

Figure 2: Photon energy versus mass ratio. The stars indicate the positions of the K X-ray fluorescence lines (see text).

In the following, we shall consider only binary reactions (reactions with only 2 heavy fragments in the exit channel). Following du Rietz et al. (2013), binary reactions are selected from the correlation plot between the fragment velocities parallel and perpendicular to the beam axis. In addition, elastic and weakly inelastic reactions are removed by requiring total center-of-mass kinetic energies smaller than , being the total energy from Viola et al. (1985), adapted for asymmetric fissions. Figure 2 presents the correlation between the photon energy and the mass ratio R = A/(A+A), where A (A) is the fragment mass in MWPC2 (MWPC1). The picture is not perfectly symmetric with respect to R = 0.5 due to efficiency losses for folding angles at R. The photon energies have been corrected for Doppler shift assuming emission from the heaviest of the 2 fragments, whatever R. Despite the selection of inelastic reactions, the different uranium peaks already observed in Fig. 1 are still dominant for mass ratios close to those for the target or projectile nucleus (R or 0.17). For intermediate R values, the Doppler correction reveals lines at constant photon energies. The stars superimposed on Fig. 2 indicate the tabulated K X-ray energies for Z, positioned at R values corresponding to neutron numbers N = Z, where the subscript T refers to the target nucleus. The positions of the stars and of the maxima of the photon lines are quite similar, indicating thus that the latter result essentially from K X-ray fluorescence.

For the Z range covered in Fig. 2, K(Z) and K(Z+1) rays can have energy differences smaller than the experimental resolution and thus cannot be separated. In order to extract the contributions of each element to the lines observed in Fig. 2, photon energy spectra have been constituted for bins of fragment masses and fits have been performed with a sum of gaussian distributions representing K and K emission from all possible elements in the energy range considered (K lines contribute only weakly to the total spectra and at energies above the K ones). Figure 3 presents as an example the Doppler corrected spectrum after background and random coincidence subtractions for fragments with mass (R). The red solid line shows the best fit, whereas the dashed (dotted) lines correspond for each Z to the K (K) contributions to this fit. All parameters were allowed to vary freely for fits to mass cuts with A , whereas, due to lower statistics, the ratios between the K and K yields had to be fixed for A at the values for diagram lines in order to reach satisfactory fits. For each Z involved, all the best fits lead both for K and K lines at the tabulated energies ( keV), with variances eV. Furthermore, for A they lead, within the statistical errors, to KK ratios in agreement with the ratios for diagram lines Kortright and Thomson (2009), as expected from the conclusions of Fig. 1 and from Behncke et al. (1979). Therefore, as exemplified by Fig. 3, the good behavior of all these fits as well in regions where only either a K or a K line is dominant as in regions where they have similar weights provides us with good confidence in the yields inferred for each Z.

The K vacancies responsible for X-ray fluorescence from the heavy QF atoms (with a fluorescence yield close to 1) are essentially created during the collision by direct interactions Reinhard et al. (1985) or later by internal conversion processes (IC). Other creation mechanisms like electron shake-off are much less probable and can be neglected Carlson et al. (1968). For QF reactions, the direct vacancies can be created as well in the incoming as in the outgoing part of the interaction and their probability depends thus slightly on the emerging fragments. Nevertheless, the narrow mass ranges considered in the following imply narrow Z ranges and similar energy distributions, leading to similar K-vacancy creation probabilities. Therefore, the total number of direct K-vacancies is actually proportional to the number of K-vacancies present at scission. The very short QF lifetime (typically up to 10 zs du Rietz et al. (2013)) does not permit the decay of these vacancies that are all quasi-adiabatically transferred to the heavier fragment, as demonstrated by molecular orbital theory Reinhard et al. (1985); Anholt (1985). The Z distributions at scission can thus be inferred from the characteristic X-ray yields resulting from direct interactions. By contrast, the number of vacancies arising from IC depends strongly on the final isotopes, after neutron evaporation, and their contributions must be subtracted from the measured X-ray yields. IC contributions have been calculated for all the known - rays in NUDAT2 extracted from the NuDat 2 database () from all the possible nuclei after evaporation (taking into account the 2.6 amu mass resolution, and between 0 and 4 neutrons emitted). Among these rays, the ones not observed (either because they are not emitted or due to too low statistics) have all been assumed to be Gaussian, with a maximum at the background level and eV, leading to a strong overestimation of their contributions. From the -ray yields and from the K conversion coefficients Kibédi et al. (2008), maximum uncertainties on the Z yields at scission have been determined.

Figure 3: Doppler corrected photon energy spectrum (histogram). The full red line is a fit to the data. The different contributions to this fit are shown by dotted and dashed lines (see text for details).

In order to check a possible effect of instrumental electronic non-linearities on the measured masses, the mass distributions obtained when the heavier QF fragment is detected either in MWPC2 or in MWPC1 have been compared for selections of characteristic X-rays associated with a restricted number of elements. For a given photon selection, provided the electronic chains have good linearities, these 2 mass distributions must have identical maxima and widths since the X-rays are emitted by the same ions. Differences of at most 1 amu for the maxima and similar widths have been found in the whole mass range involved, confirming therefore a precision on the mass identification better than 1 amu.

Figure 4: Yield, most probable atomic number and neutron number versus mass. The vertical full bars are the statistical errors. The vertical dashed lines show the maximum uncertainties resulting from internal conversion processes (see text for details).

Figure 4 presents the yield, the most probable atomic number at scission and the corresponding neutron number as a function of the fragment mass at scission. The horizontal full lines show the mass range on which the most probable Z have been determined. The latter are determined with good precision in most of the cases for A, whereas, due to statistics, larger uncertainties are obtained for A . As expected for QF, the maximum yield is found for weak mass transfers between the target and the projectile, but a secondary maximum is observed at A = 212 indicated by a dotted vertical line that crosses the data in the mid panel in the vicinity of the proton shell closure Z = 82. By contrast, it crosses the data in the lower panel at N , and the shell closure at N = 126 would rather correspond to A 206, away from the maximum yield even taking into account the statistical uncertainties. Furthermore, on the broad range 200 A, the influence of the proton shell closure seems to be felt in the mid panel through a lower slope. The strong correlation between the maximum yield and the proton shell closure at Z = 82 is highlighted by Fig. 5 that presents the Z distribution, as inferred from the fit of the photon energy spectrum between A= 210 and 214. The statistical errors are represented by the full vertical lines. The dashed lines indicate the maximum uncertainties resulting from IC for Z = 81, 82 and 83. Due to the very long computational time required to take into account all the possible converted lines, IC contributions have not been calculated for the other Z but, as indicated by vertical arrows, they can only decrease the count numbers and the most probable atomic number associated with the maximum yield is found unambiguously at Z = 82. If the neutron shell closure played a dominant role, the most probable Z would be between 84 (for A= 210) and 88 (for A=214). Maximum yields around A = 208 have been already observed and analysed Aritomo (2009); Wakhle et al. (2014); Kozulin et al. (2016) for QF experiments where only A was measured. They were interpreted either as arising from the N = 126 neutron shell closure Kozulin et al. (2016) or, according to TDHF calculations that do predict accumulations of fragments with Z , from the proton shell closure Wakhle et al. (2014). The simultaneous A and Z measurement provides thus a clear evidence for a dominant effect of the closed shell at Z = 82 on the QF fragment yield. More exclusive experiments are now needed to determine if the maximum yield results from magic number influence during the primary QF fragment formation or from enhanced stability with respect to fission of primary fragments with Z .

The present experimental approach can be applied to various systems, with or without closed shells, varying the entrance channel mass and charge asymmetries, the projectile kinetic energy, the deformations of the partners…The results should provide for theoretical models realistic controls of the neutron and proton transfers between the partners, leading thus to better predictive powers both for super-heavy synthesis by fusion and for new heavy isotope creation by transfers. It must be stressed that such experiments should also provide, besides their contribution in the super-heavy domain, quite valuable information on the symmetry energy as used in nuclear equation of state Shi and Danielewicz (2003); Chen et al. (2005); Baran et al. (2005).

Figure 5: Atomic number distribution for the quasi-fission fragments with (see text for details).

Triangles and circles in Fig. 4 show the result of TDHF calculations for central collisions for tip and side target orientation (see supplemental material Supmat ()) and different energies (simulating for a fixed bombarding energy different angular momenta, see Supmat ()). They confirm important shell effects in the Pb region with the tip orientation. The neutron and proton numbers are relatively well predicted whatever the calculated mass transfers, a quantity that reflects the most probable sticking time du Rietz et al. (2013). However, the number of protons (neutrons) is always slightly overestimated (underestimated), leading to N/Z values lower than the experimental ones for the heavier QF fragments (and thus higher for the lighter fragments). An overestimation of the N/Z equilibration present in TDHF Simenel et al. (2001); *sim07 might explain these differences. A similar behavior with respect to the data is obtained from raw static energy minimizations performed as a function of the mass asymmetry but the N/Z values for weak mass transfers are slightly lower for the heavy QF fragment than the TDHF ones, most likely due to dynamical effects in TDHF.

The simultaneous measurement of the atomic number and of the mass of quasi-fission fragments over a broad angular range demonstrates the important role played in the final fragment production by the proton shell closure at Z = 82. Further experiments are now required in order to determine if the dynamical evolution of the composite system in quasi-fission is sensitive to the shell effects of each of the individual final fragments (as predicted by TDHF microscopic calculations) or if sequential fission processes favor the survival of nuclei with magic proton numbers. The faster N/Z equilibration reached in the calculations might stress an intrinsic limitation to the TDHF approach, possibly due to the symmetry energy (and its density dependence) of the Skyrme energy density used Ka-Hae et al. (1997). In the experimental approach followed for the first time here, the uncertainties arising from internal conversion processes can be greatly reduced by reasonable increases of statistics, giving then access to the atomic number distribution for each fragment mass. X-ray fluorescence coupled with accurate mass determination opens thus a broad field of investigations of both quasi-fission and hot fission processes.

The authors warmly thank N. Lobanov, T. Kibédi, and all the accelerator staff of the ANU Heavy Ion Accelerator for their crucial technical help. The authors acknowledge support from the Australian Research Council through Discovery Grants No. FL110100098, FT120100760, DP130101569, DE140100784, DP160101254, and DP170102318. Support for accelerator operations through the NCRIS program is acknowledged. Two of us (CS and MA) acknowledge support from the Scientific Mobility Program of the Embassy of France in Australia. This research was undertaken with the assistance of resources from the National Computational Infrastructure (NCI), which is supported by the Australian Government.


  • Peter et al. (1975) J. Peter, C. Ngo,  and B. Tamain, Nuclear Physics A A250, 351 (1975).
  • Bock et al. (1982) R. Bock, Y. Chu, M. Dakowski, A. Gobbi, E. Grosse, A. Olmi, H. Sann, D. Schwalm, U. Lynen, W. Muller, S. Bjornholm, H. Esbensen, W. Wolfli,  and E. Morenzoni, Nuclear Physics A A388, 334 (1982).
  • Toke et al. (1985) J. Toke, R. Bock, G. Dai, A. Gobbi, S. Gralla, K. Hildenbrand, J. Kuzminski, W. Muller, A. Olmi, H. Stelzer, B. Back,  and S. Bjornholm, Nuclear Physics A A440, 327 (1985).
  • Back (1985) B. Back, Phys. Rev. C (Nuclear Physics) 31, 2104 (1985).
  • Morjean et al. (2008) M. Morjean, D. Jacquet, J. Charvet, A. L’Hoir, M. Laget, M. Parlog, A. Chbihi, M. Chevallier, C. Cohen, D. Dauvergne, R. Dayras, A. Drouart, C. Escano-Rodriguez, J. Frankland, R. Kirsch, P. Lautesse, L. Nalpas, C. Ray, C. Schmitt, C. Stodel, L. Tassan-Got, E. Testa,  and C. Volant, Physical Review Letters 101, 072701 (2008).
  • Frégeau et al. (2012) M. Frégeau, D. Jacquet, M. Morjean, E. Bonnet, A. Chbihi, J. Frankland, M. Rivet, L. Tassan-Got, F. Dechery, A. Drouart, L. Nalpas, X. Ledoux, M. Parlog, C. Ciortea, D. Dumitriu, D. Fluerasu, M. Gugiu, F. Gramegna, V. Kravchuk, T. Marchi, D. Fabris, A. Corsi,  and S. Barlini, Physical Review Letters 108, 122701 (2012).
  • Jacquet and Morjean (2009) D. Jacquet and M. Morjean, Progress in Particle and Nuclear Physics 63, 155 (2009).
  • Materna et al. (2004) T. Materna, Y. Aritomo, N. Amar, A. Bogatchev, V. Bouchat, O. Dorvaux, G. Giardina, S. Gre´vy, F. Hanappe, I. Itkis, M. Jandel, G. Knyajeva, J. Kliman, E. Kozulin, N. Kondratiev, L. Krupa, J. Pe´ter, E. Prokhorova, I. Pokrovsky, C. Schmitt, L. Stuttge´,  and V. Voskresensky, Nuclear Physics A 734, 184 (2004), proceedings of the Eighth International Conference On Nucleus-Nucleus Collisions.
  • Berriman et al. (2001) A. C. Berriman, D. J. Hinde, M. Dasgupta, C. R. Morton, R. D. Butt,  and J. O. Newton, Nature 413, 144 (2001).
  • Hinde et al. (2008a) D. J. Hinde, R. du Rietz, M. Dasgupta, R. G. Thomas,  and L. R. Gasques, Phys. Rev. Lett. 101, 092701 (2008a).
  • Hinde et al. (2008b) D. J. Hinde, R. G. Thomas, R. du Rietz, A. Diaz-Torres, M. Dasgupta, M. L. Brown, M. Evers, L. R. Gasques, R. Rafiei,  and M. D. Rodriguez, Phys. Rev. Lett. 100, 202701 (2008b).
  • Nishio et al. (2012) K. Nishio, S. Mitsuoka, I. Nishinaka, H. Makii, Y. Wakabayashi, H. Ikezoe, K. Hirose, T. Ohtsuki, Y. Aritomo,  and S. Hofmann, Phys. Rev. C 86, 034608 (2012).
  • du Rietz et al. (2013) R. du Rietz, E. Williams, D. J. Hinde, M. Dasgupta, M. Evers, C. J. Lin, D. H. Luong, C. Simenel,  and A. Wakhle, Phys. Rev. C 88, 054618 (2013).
  • Williams et al. (2013) E. Williams, D. Hinde, M. Dasgupta, R. du Rietz, I. Carter, M. Evers, D. Luong, S. McNeil, D. Rafferty, K. Ramachandran,  and A. Wakhle, Physical Review C (Nuclear Physics) 88, 034611 (2013).
  • Wakhle et al. (2014) A. Wakhle, C. Simenel, D. J. Hinde, M. Dasgupta, M. Evers, D. H. Luong, R. du Rietz,  and E. Williams, Phys. Rev. Lett. 113, 182502 (2014).
  • Kozulin et al. (2016) E. M. Kozulin, G. N. Knyazheva, K. V. Novikov, I. M. Itkis, M. G. Itkis, S. N. Dmitriev, Y. T. Oganessian, A. A. Bogachev, N. I. Kozulina, I. Harca, W. H. Trzaska,  and T. K. Ghosh, Phys. Rev. C 94, 054613 (2016).
  • Prasad et al. (2016) E. Prasad, A. Wakhle, D. J. Hinde, E. Williams, M. Dasgupta, M. Evers, D. H. Luong, G. Mohanto, C. Simenel,  and K. Vo-Phuoc, Phys. Rev. C 93, 024607 (2016).
  • Sekizawa and Yabana (2016) K. Sekizawa and K. Yabana, Phys. Rev. C 93, 054616 (2016).
  • Li et al. (2016) C. Li, F. Zhang, J. Li, L. Zhu, J. Tian, N. Wang,  and F.-S. Zhang, Phys. Rev. C 93, 014618 (2016).
  • Oberacker et al. (2014) V. E. Oberacker, A. S. Umar,  and C. Simenel, Phys. Rev. C 90, 054605 (2014).
  • Umar et al. (2015) A. Umar, V. Oberacker,  and C. Simenel, Physical Review C (Nuclear Physics) 92, 024621 (2015).
  • Umar et al. (2016) A. Umar, V. Oberacker,  and C. Simenel, Physical Review C 94, 024605 (2016).
  • Simenel et al. (2012) C. Simenel, D. Hinde, R. du Rietz, M. Dasgupta, M. Evers, C. Lin, D. Luong,  and A. Wakhle, Physics Letters B 710, 607 (2012).
  • Simenel (2012) C. Simenel, The European Physical Journal A 48, 152 (2012).
  • Diaz-Torres et al. (2001) A. Diaz-Torres, G. G. Adamian, N. V. Antonenko,  and W. Scheid, Phys. Rev. C 64, 024604 (2001).
  • Zagrebaev and Greiner (2007) V. Zagrebaev and W. Greiner, J. Phys. G: Nuclear and Particle Physics 34, 1 (2007).
  • Aritomo et al. (2012) Y. Aritomo, K. Hagino, K. Nishio,  and S. Chiba, Phys. Rev. C 85, 044614 (2012).
  • Enqvist et al. (2001) T. Enqvist, W. Wlazło, P. Armbruster, J. Benlliure, M. Bernas, A. Boudard, S. Czajkowski, R. Legrain, S. Leray, B. Mustapha, M. Pravikoff, F. Rejmund, K.-H. Schmidt, C. Stéphan, J. Taieb, L. Tassan-Got,  and C. Volant, Nuclear Physics A 686, 481 (2001).
  • Armbruster et al. (2004) P. Armbruster, J. Benlliure, M. Bernas, A. Boudard, E. Casarejos, S. Czajkowski, T. Enqvist, S. Leray, P. Napolitani, J. Pereira, F. Rejmund, M.-V. Ricciardi, K.-H. Schmidt, C. Stéphan, J. Taieb, L. Tassan-Got,  and C. Volant, Phys. Rev. Lett. 93, 212701 (2004).
  • Caamaño et al. (2013) M. Caamaño, O. Delaune, F. Farget, X. Derkx, K.-H. Schmidt, L. Audouin, C.-O. Bacri, G. Barreau, J. Benlliure, E. Casarejos, A. Chbihi, B. Fernández-Domínguez, L. Gaudefroy, C. Golabek, B. Jurado, A. Lemasson, A. Navin, M. Rejmund, T. Roger, A. Shrivastava,  and C. Schmitt, Phys. Rev. C 88, 024605 (2013).
  • Martin et al. (2015) J.-F. Martin, J. Taieb, A. Chatillon, G. Bélier, G. Boutoux, A. Ebran, T. Gorbinet, L. Grente, B. Laurent, E. Pellereau, H. Alvarez-Pol, L. Audouin, T. Aumann, Y. Ayyad, J. Benlliure, E. Casarejos, D. Cortina Gil, M. Caamaño, F. Farget, B. Fernandez Dominguez, A. Heinz, B. Jurado, A. Kelic-Heil, N. Kurz, C. Nociforo, C. Paradela, S. Pietri, D. Ramos, J.-L. Rodriguez-Sanchez, C. Rodriguez-Tajes, D. Rossi, K.-H. Schmidt, H. Simon, L. Tassan-Got, J. Vargas, B. Voss,  and H. Weick, EPJ A - Hadrons and Nuclei 51, 174 (2015).
  • Chebboubi et al. (2016) A. Chebboubi, G. Kessedjian, H. Faust, A. Blanc, M. Jentschel, U. Köster, T. Materna, O. Méplan, C. Sage,  and O. Serot, NIM B 376, 120 (2016).
  • Griffin (1990) H. Griffin, J. Rad. Nucl. Chem. 142, 279 (1990).
  • Kortright and Thomson (2009) J. Kortright and A. Thomson, X-ray data booklet, edited by A. Thomson, 1-8 (Lawrence Berkeley National Laboratory, 2009).
  • Behncke et al. (1979) H. H. Behncke, P. Armbruster, F. Folkmann, S. Hagmann, J. R. Macdonald,  and P. H. Mokler, Z. Phys. A 289, 333 (1979).
  • Viola et al. (1985) V. E. Viola, K. Kwiatkowski,  and M. Walker, Phys. Rev. C 31, 1550 (1985).
  • Reinhard et al. (1985) J. Reinhard, W. Greiner, J. Greenbergand,  and P. Vincent, Treatise on Heavy-Ion Science, edited by A. Bromley, Vol. 5 (Plenum, New York, 1985).
  • Carlson et al. (1968) T. A. Carlson, C. W. Nestor, T. C. Tucker,  and F. B. Malik, Phys. Rev. 169, 27 (1968).
  • Anholt (1985) R. Anholt, Rev. Mod. Phys. 57, 995 (1985).
  • (40) NUDAT2, National Nuclear Data Center, Information extracted from the NuDat 2 database, http://www.nndc.bnl.gov/nudat2/ .
  • Kibédi et al. (2008) T. Kibédi, T. Burrows, M. Trzhaskovskaya, P. Davidson,  and C. N. Jr., NIM A 589, 202 (2008).
  • Aritomo (2009) Y. Aritomo, Phys. Rev. C 80, 064604 (2009).
  • Shi and Danielewicz (2003) L. Shi and P. Danielewicz, Phys. Rev. C 68, 064604 (2003).
  • Chen et al. (2005) L.-W. Chen, C. M. Ko,  and B.-A. Li, Phys. Rev. Lett. 94, 032701 (2005).
  • Baran et al. (2005) V. Baran, M. Colonna, M. D. Toro, M. Zielinska-Pfabé,  and H. H. Wolter, Phys. Rev. C 72, 064620 (2005).
  • (46) See Supplemental Material for TDHF calculations .
  • Simenel et al. (2001) C. Simenel, P. Chomaz,  and G. de France, Physical Review Letters 86, 2971 (2001).
  • Simenel et al. (2007) C. Simenel, P. Chomaz,  and G. de France, Physical Review C (Nuclear Physics) 76, 024609 (2007).
  • Ka-Hae et al. (1997) K. Ka-Hae, T. Otsuka,  and P. Bonche, in Journal of Physics G (Nuclear and Particle Physics), Vol. 23 (Dept. of Phys., Tokyo Univ., Japan, 1997) pp. 1267 – 1273.
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